scispace - formally typeset
P

Pablo Martínez-Miravé

Researcher at University of Valencia

Publications -  13
Citations -  551

Pablo Martínez-Miravé is an academic researcher from University of Valencia. The author has contributed to research in topics: Neutrino oscillation & Neutrino. The author has an hindex of 4, co-authored 9 publications receiving 217 citations. Previous affiliations of Pablo Martínez-Miravé include Spanish National Research Council.

Papers
More filters
Journal ArticleDOI

2020 global reassessment of the neutrino oscillation picture

TL;DR: In this article, the authors presented an updated global fit of neutrino oscillation data in the simplest three-neutrino framework, which showed a strong preference for the normal neutrinos mass ordering with 25σ statistical significance.
Journal ArticleDOI

2020 Global reassessment of the neutrino oscillation picture

TL;DR: In this paper, the authors presented an updated global fit of neutrino oscillation data in the simplest three-neutrino framework and showed that there is a strong agreement between the Bayesian and frequentist approaches.
Journal ArticleDOI

Signatures of ultralight dark matter in neutrino oscillation experiments

TL;DR: In this article, three distinct signatures on neutrino oscillations are identified, depending on the mass of the dark matter and the specific experimental setup, which are time modulation signals, oscillation probability distortions due to fast modulations, and fast varying matter effects.
Journal ArticleDOI

Signatures of primordial black hole dark matter at DUNE and THEIA

TL;DR: In this paper, the authors explore the possibility of detecting light (non-)rotating primordial black holes (PBHs) with future neutrino experiments, and they focus on two next generation facilities: the Deep Underground Neutrino Experiment (DUNE) and THEIA.
Journal ArticleDOI

Signatures of Ultralight Dark Matter in Neutrino Oscillation Experiments

TL;DR: In this article, three distinct signatures on neutrino oscillations are identified, depending on the mass of the dark matter and the specific experimental setup, which are time modulation signals, oscillation probability distortions due to fast modulations, and fast varying matter effects.